来自 (α,n) 反应的优化中子产量计算,使用修改的SOURCES4代码
M Parvu1, P Krawczun2, V A Kudryavtsev2
1Faculty of Physics, University of Bucharest, POBox 11, 077125, Magurele, Romania.
概括
这项研究改进了用于罕见事件搜索的中子背景计算. 使用更新的α-中子 (α,n) 反应截面的新计算提高了暗物质和中微子实验的准确性.
科学领域:
- 核物理学 核物理 核物理
- 粒子物理学的粒子物理学.
- 天体物理学 天体物理学
背景情况:
- 对于罕见事件 (暗物质,中微子) 的地下实验受到中子背景的限制.
- 中子起源于自发的裂变和α-中子 (α,n) 反应.
- 精确的中子产量和能量光谱计算对于灵敏度至关重要.
研究的目的:
- 使用修改后的SOURCES4代码,呈现新的中子生产计算.
- 将 (α,n) 反应的更新截面纳入.
- 将计算结果与实验数据进行比较.
主要方法:
- 使用修改后的SOURCES4代码进行中子生成计算.
- 整合了最近更新的 (α,n) 反应的实验截面.
- 在实验数据有限的情况下,补充了EMPIRE,TALYS和JENDL-5计算.
主要成果:
- 根据精制的 (α,n) 截面提出了新的中子产生计算.
- 计算与阿尔法光束和放射性衰变的现有实验数据之间的一致性.
- 确定了可靠的截面,用于准确的中子背景估计.
结论:
- 更新的SOURCES4代码与新的截面提供了更准确的中子背景预测.
- 这些改进的计算对于提高罕见事件搜索实验的灵敏度至关重要.
- 该研究提供了一种经过验证的方法,用于在核天体物理学和粒子物理学研究中选择可靠的横截面.
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